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NASA发表研究报告分析生命在木星卫星上存在所需的化学条件

(2013-04-16 11:09:02)
标签:

杂谈

分类: 科学与技术

http://photos.state.gov/libraries/amgov/3234/week_2/04082013_jupiter_moon_jpg_600.jpg

2013.04.10

根据最近发表的一篇研究报告,在木星(Jupiter)卫星木卫二(Europa)的整个表面分布着大量的过氧化氢。研究报告的作者认为,如果木卫二表面的过氧化氢下面的海洋混合,就可能为将来可能出现的简单生命形式提供重要的能量来源。

根据最近发表的一篇研究报告,在木星(Jupiter)卫星木卫二(Europa)的整个表面分布着大量的过氧化氢。研究报告的作者认为,如果木卫二表面的过氧化氢下面的海洋混合,就可能为将来可能出现的简单生命形式提供重要的能量来源。这篇文章最近发表在《天体物理杂志通讯》(Astrophysical Journal Letters)网络版上。

研究报告的主要作者凯文·汉德(Kevin Hand)在加利福尼亚州帕萨迪纳(Pasadena, California)的美国国家航空航天局(NASA)喷气推进实验室(Jet Propulsion Laboratory)工作。他说:“我们所了解的生命需要液态水及碳、氮、磷和硫等元素,并需要某种形式的化学或光能,这样才能形成生命。木卫二有液态水和这些元素,而且我们认为,像过氧化氢之类的化合物可能是满足能源要求的重要成分。地球具备过氧化物等氧化剂,为复杂、多细胞生命出现提供了一个关键的条件。”

这项研究由美国国家航空航天局天体生物学研究所(NASA Astrobiology Institute)提供部分资助,并由设在喷气推进实验室的冰雪世界(Icy Worlds)团队完成。美国国家航空航天局天体生物学研究所是美国国家航空航天局、15个美国研究团队和13个国际联合团队共同建立的伙伴机构。

上图是木卫二的紫色、绿色和红外图像的彩色复合图,左图是该卫星的自然色彩图,右图是为突出其表面的细微颜色差别制作的重彩图。木卫二表面的亮白色和蓝色部分主要由水冰组成,



Read more: http://iipdigital.usembassy.gov/st/chinese/inbrief/2013/04/20130410145557.html#ixzz2QamOX0s8

http://photos.state.gov/libraries/amgov/3234/week_2/04082013_jupiter_moon_jpg_600.jpg

09 April 2013

A new paper shows that hydrogen peroxide is abundant across much of the surface of Jupiter's moon Europa. The authors argue that if the peroxide on the surface of Europa mixes into the ocean below, it could be an important energy supply for simple forms of life, if life were to exist there.

A new paper shows that hydrogen peroxide is abundant across much of the surface of Jupiter's moon Europa. The authors argue that if the peroxide on the surface of Europa mixes into the ocean below, it could be an important energy supply for simple forms of life, if life were to exist there. The paper was published online recently in the Astrophysical Journal Letters.

“Life as we know it needs liquid water, elements like carbon, nitrogen, phosphorus and sulfur, and it needs some form of chemical or light energy to get the business of life done," said Kevin Hand, the paper's lead author, based at NASA's Jet Propulsion Laboratory (JPL), Pasadena, California. “Europa has the liquid water and elements, and we think that compounds like peroxide might be an important part of the energy requirement. The availability of oxidants like peroxide on Earth was a critical part of the rise of complex, multicellular life.”

The study was funded in part by the NASA Astrobiology Institute through the Icy Worlds team based at JPL. The NASA Astrobiology Institute is a partnership among NASA, 15 U.S. teams and 13 international consortia.

This color composite view above combines violet, green, and infrared images of Europa for a view of the moon in natural color (left) and in enhanced color designed to bring out subtle color differences in the surface (right). The bright white and bluish part of Europa's surface is composed mostly of water ice, with very few non-ice materials. In contrast, the brownish mottled regions on the right side of the image may be covered by hydrated salts and an unknown red component.



Read more: http://iipdigital.usembassy.gov/st/english/inbrief/2013/04/20130407145370.html#ixzz2QamPkaMf

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